Results 31 to 40 of about 26,635,104 (298)

Lunin-Maldacena backgrounds from the classical Yang-Baxter equation - Towards the gravity/CYBE correspondence [PDF]

open access: yes, 2014
We consider γ-deformations of the AdS5×S5 superstring as Yang-Baxter sigma models with classical r-matrices satisfying the classical Yang-Baxter equation (CYBE).
Kentaroh Yoshida   +5 more
core   +2 more sources

STUDY OF SYMMETRY IN F(R) THEORY OF GRAVITY [PDF]

open access: yesModern Physics Letters A, 2010
An action in which the Ricci scalar is non-minimally coupled with a scalar field and contains higher order curvature invariant terms carries a conserved current under certain conditions that decouples geometric part from the scalar field. The conserved current relates the pair of arbitrary coupling parameters f(ϕ) and ω(ϕ) with the gravitational field
openaire   +3 more sources

Higher-derivative f(R,□R,T) theories of gravity [PDF]

open access: yesInternational Journal of Modern Physics D, 2017
In literature, there is a model of modified gravity in which the matter Lagrangian is coupled to the geometry via trace of the stress–energy–momentum tensor [Formula: see text]. This type of modified gravity is denoted [Formula: see text] in which [Formula: see text] is Ricci scalar [Formula: see text].
Houndjo, M. J. S.   +4 more
openaire   +2 more sources

EMERGENT UNIVERSE IN THE CHAMELEON, f(R) AND f(T) GRAVITY THEORIES [PDF]

open access: yesInternational Journal of Modern Physics D, 2011
In this work, we consider an emergent Universe in generalized gravity theories like the chameleon, f(R) and f(T) gravities. We reconstruct the potential of the chameleon field under the emergent scenario of the Universe and observe its increasing nature with the evolution of the Universe.
Chattopadhyay, Surajit, Debnath, Ujjal
openaire   +3 more sources

The philosophy behind quantum gravity [PDF]

open access: yes, 2006
This paper investigates some of the philosophical and conceptual issues raised by the search for a quantum theory of gravity. It is critically discussed whether such a theory is necessary in the first place, and how much would be accomplished if it is ...
Zinkernagel, Henrik   +2 more
core   +1 more source

Charged wormholes in f(R,T)-extended theory of gravity [PDF]

open access: yesInternational Journal of Modern Physics D, 2019
Wormholes (WHs) are a solution for General Relativity field equations which characterize a passage or tunnel that connects two different regions of spacetime and is filled by some sort of exotic matter that does not satisfy the energy conditions. On the other hand, it is known that in extended theories of gravity, the extra degrees of freedom once ...
P. H. R. S. Moraes   +2 more
openaire   +2 more sources

ENERGY CONDITIONS IN f(R) GRAVITY AND BRANS–DICKE THEORIES [PDF]

open access: yesInternational Journal of Modern Physics D, 2009
The equivalence between f(R) gravity and scalar–tensor theories is invoked to study the null, strong, weak and dominant energy conditions in Brans–Dicke theory. We consider the validity of the energy conditions in Brans–Dicke theory by invoking the energy conditions derived from a generic f(R) theory. The parameters involved are shown to be consistent
Atazadeh, K.   +3 more
openaire   +3 more sources

Ghost-free F(R) gravity with Lagrange multiplier constraint

open access: yesPhysics Letters B, 2017
We propose two new versions of ghost-free generalized F(R) gravity with Lagrange multiplier constraint. The first version of such theory for a particular degenerate choice of the Lagrange multiplier, corresponds to mimetic F(R) gravity.
S. Nojiri, S.D. Odintsov, V.K. Oikonomou
doaj   +1 more source

Neutron stars in $$f(\mathtt {R,L_m})$$ f ( R , L m ) gravity with realistic equations of state: joint-constrains with GW170817, massive pulsars, and the PSR J0030+0451 mass-radius from NICER data

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
In this work, we investigate neutron stars (NS) in $$f(\mathtt {R,L_m})$$ f ( R , L m ) theory of gravity for the case $$f(\mathtt {R,L_m})= \mathtt {R}+ \mathtt {L_m}+ \sigma \mathtt {R}\mathtt {L_m}$$ f ( R , L m ) = R + L m + σ R L m , where $$\mathtt
R. V. Lobato   +2 more
doaj   +1 more source

Redundant operators in the exact renormalisation group and in the f(R) approximation to asymptotic safety

open access: yes, 2013
In this paper we review the definition and properties of redundant operators in the exact renormalisation group. We explain why it is important to require them to be eigenoperators and why generically they appear only as a consequence of symmetries of ...
Morris, Tim R., Dietz, Juergen A.
core   +1 more source

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